Three-dimensional simulations of solar wind turbulence with the hybrid code CAMELIA (2018)
Attributed to:
Solar and Planetary Research at Queen Mary 2017-2020
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1088/1742-6596/1031/1/012002
Publication URI: http://dx.doi.org/10.1088/1742-6596/1031/1/012002
Type: Journal Article/Review
Parent Publication: Journal of Physics: Conference Series